CWNU 3144

0.36 UTI

0.5

C_N

0.56

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 50

Radius (P>50% members) 1.3 [arcmin]

C_N 0.5 Moderately populated
C_dens 0.56 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3144 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~11.19 kpc) differs significantly from the median photometric distance (~7.76 kpc).

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3144 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	102.849	-14.531	0.089	-0.19	1.1	102.501
He et al.	2023	102.853	-14.523	0.085	-0.199	1.069	92.77

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
He et al.	2023	7.76	1.25	–	251	–	–	–	–

Visualization

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